|Veröffentlichungsdatum||7. Febr. 2017|
|Eingetragen||21. Apr. 2015|
|Prioritätsdatum||7. Juli 2010|
|Auch veröffentlicht unter||CN103155451A, EP2591565A1, US9048950, US20120008961, US20150349888, WO2012006209A1|
|Veröffentlichungsnummer||14692583, 692583, US 9564968 B2, US 9564968B2, US-B2-9564968, US9564968 B2, US9564968B2|
|Erfinder||Young-Kai Chen, Noriaki Kaneda, Alex Pidwerbetsky|
|Ursprünglich Bevollmächtigter||LGS Innovations LLC|
|Zitat exportieren||BiBTeX, EndNote, RefMan|
|Patentzitate (44), Nichtpatentzitate (2), Klassifizierungen (5)|
|Externe Links: USPTO, USPTO-Zuordnung, Espacenet|
This application is a continuation of U.S. application Ser. No. 12/915,506, filed on Oct. 29, 2010, which claims priority to U.S. Provisional Application No. 61/362,201, filed on Jul. 7, 2010, and is related to International Application No. PCT/US2011/042562, filed on Jun. 30, 2011, the disclosures of which are incorporated herein by reference in their entirety.
This invention relates to free-space optical communication.
The advantages of free-space optical communication (FSO), such as high bandwidth and high signal directivity, have long been known. One of the known drawbacks of FSO is its susceptibility to scintillation. That is, turbulence and thermal phenomena create localized fluctuations in the atmospheric refractive index. A signal-carrying FSO beam passing through such fluctuations may be wholly or partially deflected due to optical refraction. One consequence is that at the receiving end, where the beam is focused onto an image spot, the image spot may wander in the image plane.
Moreover, FSO beams are typically generated as coherent laser beams. A coherent beam initially has a uniform wavefront, i.e., a phase that varies slowly with radial position over the leading face of the beam. A beam having a uniform wavefront is desirable because at the detector, it will experience relatively little destructive self-interference. However, a second effect of index fluctuations in the atmosphere is to distort the wavefront of the FSO beam. The distortions cause time-dependent, destructive self-interference of the beam at the detector, which leads, in turn, to fading of the received signal.
Some of the known solutions to the problems related to atmospheric scintillation use mechanical mirrors and adaptive optics to track the wandering beam and to correct the distorted wavefront. However, such solutions require bulky hardware components. Some of them also use a closed, iterative control loop of sensing and mechanical actuation that limits their performance. These drawbacks are particularly severe in the case of QAM and other advanced modulation methods for the FSO beam, for which reception is relatively sensitive to the fidelity of the amplitude and phase of the received signal.
We have provided a new solution, which makes use of the fact that different wavelengths will generally exhibit different fading characteristics in a propagation environment characterized by atmospheric scintillation. Our solution offers the possibility of open-loop adaptive processing that may be done purely in high-speed electronics. This allows for coherent processing across the wavefront and enables optical MIMO by taking advantage of the multipath propagation produced by the atmosphere.
In an embodiment, our solution involves collecting at least one FSO beam, demultiplexing the beam, by wavelength, into at least two sub-beams, detecting each sub-beam to produce an electrical output therefrom, and recovering a signal using complementary information from at least two of the electrical outputs.
Although only a single projected, wavelength-multiplexed output beam 50 is shown for simplicity of presentation, it will be understood that some advantages of spatial diversity may be achieved through arrangements in which multiple wavelength-multiplexed output beams are produced. This may be done, for example, by using multiple transmit apertures.
Numerous alternative implementations of the system shown conceptually in
Preferred methods of data encoding for optical transmission rates of 10 Gbps and above include PSK, QAM, and OFDM. Additionally, it may be advantageous in at least some cases to employ space-time block codes and the like, in which the coded constellation symbols are arranged in space-time matrices or wavelength-time matrices, or over matrices that extend in space, time, and wavelength. (A space-time matrix distributes the signal over multiple output sub-apertures and multiple symbol intervals. A wavelength-time matrix distributes the signal over multiple wavelength subchannels and multiple symbol intervals.)
Numerous alternative implementations of the system shown conceptually in
As seen in the figure, the DSP has multiple input streams, each corresponding to one of the wavelength channels that are demultiplexed into respective sub-beams. The DSP uses complementary information from at least two, and preferably from all, of these wavelength channels in order to compute the output data stream 120.
For example, redundant information may be sent on each of two or more wavelength channels. In such a case, the DSP may select for a period of time that wavelength channel (or that subset of wavelength channels) that is strongest. By “strongest” is meant that which affords the greatest probability of accurate reception. Strength may be measured by signal-to-noise ratio, by error probability as determined from pilot signals sent on the pertinent wavelength channel, or by other well-known means. The period of time during which a particular channel selection persists may be determined, for example, by measurements of the coherence time of the propagation environment, which in some cases may be several milliseconds. According to such an approach, the information in different wavelength channels is “complementary” in the sense that the same information that is received weakly in one channel may be received more strongly in another.
Information in different wavelength channels may also be “complementary” because different channels carry distinct data streams. That is, data encoder 10 of
In at least some cases, it will be advantageous for DSP 110 to implement a diversity receiver. In a diversity receiver, the respective data streams 130.1, . . . , 130.n that are input to the DSP are assigned different weights. The set of weights is computed to minimize an error probability, based on pilot signals received from the transmitter. In such a case, the information on the different frequency channels is “complementary” because when combined in the DSP according to its assigned weight, each channel contributes to an optimized received signal.
In at least some cases, it will be advantageous for DSP 110 to implement MIMO techniques to recover the signal from space-time matrices, frequency-time matrices, and the like. As will be discussed below, such processing may include the use of propagation coefficients obtained, for example, from measurements made using pilot signals received from the transmitter. Separate pilot signals may be sent on different wavelength channels as well as from different transmitter sub-apertures. Likewise, pilot signals may be received in different receiver sub-apertures. Accordingly, a matrix of propagation coefficients may be determined for each wavelength channel. Within each such matrix, a given coefficient expresses an attenuation and a phase delay between a given transmitter sub-aperture and a given receiver sub-aperture. The use of such matrix information will be described further, below.
In other embodiments, the tapered fiber bundle may be replaced by a single fiber tapered from a large core (at the focus of the optical telescope) to a small core, thus adiabatically guiding the light into a single-mode (small core) output fiber.
The arrangement of elements as shown in
In a broad sense, one of the principles that
Accordingly, it will be understood that it is advantageous for the entrance end of the tapered fiber or fiber bundle to have a large effective core, that a fiber bundle achieves this with a total core that is the effective sum of the cores of the constitutent fibers, and that an alternative is to use a tapered single fiber having (initially) a relatively large core. In at least some cases, the approach using a single tapered fiber may be the most advantageous because the single fiber suffers less optical loss due to the cladding covering part of the aperture. A single-fiber taper may also be simpler to fabricate, because it is free of the exacting path-length tolerances that may need to be imposed on a tapered fiber bundle in order to mitigate interference between the fibers that constitute the bundle.
As noted above, both beam wander and wavefront distortion are undesirable phenomena that tend to degrade the performance of the communication system. Wavefront distortion becomes more damaging as data rates increase, because the resulting spread in the propagating wavefront may become comparable to the spacing between successive pulses in the modulated light beam.
In order to be able to effectively mitigate the effects of wavefront distortion, it is advantageous to use an effective optical aperture for the detector that is less than one coherence length, or to subdivide the total aperture into subapertures, each having its own detector or detectors. Each subaperture is also advantageously provided with its own wavelength demultiplexer situated prior to the respective detector or detectors.
It will be seen that
In an alternative arrangement, the wavelength demultiplexer is situated downstream of the taper. In particular, it could be advantageous to situate the entrance to a single-fiber taper in a focal plane of the telescope, and to direct the collected light through the tapered fiber to a single-mode wavelength demultiplexer. Such devices are desirable because they are compact and they are readily fabricated using known techniques. Single-mode fibers can be used to route the output signals from the wavelength demultiplexer to respective photodetectors.
However, it should be noted that such an arrangement may be most suitable when wavefront distortion is of lesser concern, so that a single large aperture can be tolerated for collecting the light injected into the taper.
Cases of larger wavefront distortion can be handled by the use of multiple fiber tapers (by using, for example, a fiber taper bundle) at the focal plane of the telescope. In such cases, the multiple fiber tapers effectively divide the focal spot into a set of coherent sub-patches, each of which can be processed in the same manner as in the case of a single fiber taper. Each fiber taper is then followed by a single-mode wavelength demultiplexer and by detectors for the individual wavelengths.
Once the optical signals are converted to electrical signals, the wavefront distortion can be measured across the sub-patches and across wavelengths, and it can be corrected. This enables the implementation of adaptive optics in the electronic domain. Furthermore, such electronics-based adaptive optics is more flexible than conventional adaptive optics because it permits the amplitude and the phase to be controlled independently for each wavelength. This, in turn, enables more specific compensation for the wavefront distortions.
When operated as a transmitter, such an arrangement is one possible source (among various others) of signals carried in multiple, spatially diverse sub-beams. Spatial diversity is most effective when the separation between the effective apertures for the respective sub-beams (in either transmission or reception) is comparable to, or greater than, a pertinent coherence length. For example, the pertinent coherence length may be the coherence length of the distorted wavefront in the object or image plane, respectively, of the transmission or reception telescope.
Coherence lengths are readily computed from the theory of two-frequency mutual coherence functions in turbulent media, which is discussed below.
Those skilled in the art will appreciate further that spatial diversity may be achieved in both transmission and reception by pairing a transmitter and a receiver that both have multiple apertures according, for example, to the arrangement of
The propagation coefficients can be measured using coherent detection of optical pilot signals, according to methods well known to those versed in radiofrequency MIMO technology. Generally, the propagation coefficients may be treated as quasi-static for the coherence time of the atmospheric propagation channel.
As is well known in the field of MIMO, the optical outputs of the transmit apertures during a symbol interval may be described as a vector x, and the optical inputs at the receive apertures as a vector y. In such a notation, the coupling between each of the transmit apertures and each of the receive apertures may be described by a matrix H whose entries are the propagation coefficients hij. Accordingly, the total optical signal arriving at a given receive aperture, including the effects of optical fading caused by the phase distortions described above, may be expressed as the vector product of x (if x is taken as a row vector) times that column of H that corresponds to the given receive aperture. The same is generally true at each of the multiple receive apertures.
One consequence is that if H can be effectively inverted, the distortions caused by atmospheric turbulence (as averaged over each spatial sub-beam) can be corrected through numerical processing, and in effect, the undistorted wavefronts can be recovered. It follows that signal loss due to fading can be at least partially reversed, and a stronger signal can be recovered.
In one example, a single transmit stream is transmitted. It may be transmitted from a single transmit aperture or from multiple transmit apertures. In the case of a single transmit stream, the matrix H reduces to a single row, and the pertinent processing of the received signal is equivalent to the coherent combination of the various versions or the signal received from the respective receive apertures or subapertures. In theory, this corresponds to the result that is sought using adaptive optics. However, our approach can achieve this result without using a control loop, and it can adjust for both the amplitude and the phase of the received signals.
Furthermore, our approach can be applied in cases where the time delay due to the propagation is significant relative to the symbol duration. Such cases are not adequately treated, in general, by traditional methods of adaptive optics.
A number of techniques for achieving an effective inversion of H are well known in the field of radiofrequency MIMO, and they may also be applied to optical MIMO as described here.
The optical MIMO techniques described here may be applied in a single wavelength channel, or in any number of wavelength subchannels.
As noted above, the theory of two-frequency mutual coherence functions in turbulent media provides a framework for calculating coherence lengths. The same theory also provides a framework for calculating the coherence bandwidth (which is also referred to as the correlation or decorrelation bandwidth). For example, a theoretical calculation of the coherence bandwidth for the case of strong scintillation is given in A. Ishimaru, Wave Propagation and Scattering in Random Media, Volume 2 (1978) 424-426. A theoretical calculation for the case of weak scintillation case is given in L. Andrews and R. L. Phillips, Laser Beam Propagation through Random Media (1998) 150-152.
Those skilled in the art will appreciate that for effective operation, the spacing between the respective wavelength bands assigned to the various sub-beams should be at least the coherence bandwidth, so that wavelength-based decorrelation between sub-beams can take place. Those skilled in the art will appreciate further that the total bandwidth spanned by the sub-beams should lie within the amplification bandwidth of the receiver. Accordingly, the amplification bandwidth imposes an upper limit on the wavelength spacing.
It will be appreciated further that the coherence bandwidth depends on the average wavelength, the range (i.e., the transmission distance), and the level of turbulence in the transmission path. Thus, for a given range and turbulence level, it is advantageous to select the average wavelength such that the constraints described above can be satisfied using appropriate optical amplifiers.
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|2||Ishimaru, "Wave Propagation and Scattering in random Media", vol. 2, 1978.|
|Internationale Klassifikation||H04B10/112, H04B10/61, H04B10/00|